Matches in SemOpenAlex for { <https://semopenalex.org/work/W3105789788> ?p ?o ?g. }
- W3105789788 endingPage "26" @default.
- W3105789788 startingPage "26" @default.
- W3105789788 abstract "In this paper we collect 19 hydrogen-deficient superluminous supernovae (SLSNe) and fit their light curves, temperature evolution, and velocity evolution based on the magnetar-powered model. To obtain the best-fitting parameters, we incorporate the Markov chain Monte Carlo approach. We get rather good fits for seven events (χ2/dof = 0.24–0.96) and good fits for another seven events (χ2/dof = 1.37–3.13). We find that the initial periods (P0) and magnetic strength (Bp) of the magnetars that supposedly power these SLSNe are in the range of ∼1.2–8.3 ms and G, respectively; the inferred masses of the ejecta of these SLSNe are between 1 and , and the values of the gamma-ray opacity are between 0.01 and 0.82 cm2 g−1. We also calculate the fraction of the initial rotational energy of the magnetars harbored in the centers of the remnants of these SLSNe that is converted to the kinetic energy of the ejecta and find that the fraction is ∼19%–97% for different values of P0 and Bp, indicating that the acceleration effect cannot be neglected. Moreover, we find that the initial kinetic energies of most of these SLSNe are so small ( erg) that they can be easily explained by the neutrino-driven mechanism. These results can help clarify some important issues related to the energy-source mechanisms and explosion mechanisms and reveal the nature of SLSNe." @default.
- W3105789788 created "2020-11-23" @default.
- W3105789788 creator A5003038198 @default.
- W3105789788 creator A5030184407 @default.
- W3105789788 creator A5056472307 @default.
- W3105789788 creator A5058285440 @default.
- W3105789788 creator A5082967419 @default.
- W3105789788 creator A5088617390 @default.
- W3105789788 date "2017-06-08" @default.
- W3105789788 modified "2023-10-16" @default.
- W3105789788 title "A Monte Carlo Approach to Magnetar-powered Transients. I. Hydrogen-deficient Superluminous Supernovae" @default.
- W3105789788 cites W1861327581 @default.
- W3105789788 cites W1946870327 @default.
- W3105789788 cites W1967583406 @default.
- W3105789788 cites W1967653785 @default.
- W3105789788 cites W1976714811 @default.
- W3105789788 cites W1977925093 @default.
- W3105789788 cites W1979165635 @default.
- W3105789788 cites W1979827546 @default.
- W3105789788 cites W1992420274 @default.
- W3105789788 cites W1995299616 @default.
- W3105789788 cites W2011634292 @default.
- W3105789788 cites W2019046080 @default.
- W3105789788 cites W2038991267 @default.
- W3105789788 cites W2041791190 @default.
- W3105789788 cites W2042465048 @default.
- W3105789788 cites W2043993903 @default.
- W3105789788 cites W2047135448 @default.
- W3105789788 cites W2054185545 @default.
- W3105789788 cites W2061298785 @default.
- W3105789788 cites W2063498033 @default.
- W3105789788 cites W2073734144 @default.
- W3105789788 cites W2079603396 @default.
- W3105789788 cites W2082641261 @default.
- W3105789788 cites W2092165725 @default.
- W3105789788 cites W2092375055 @default.
- W3105789788 cites W2095319512 @default.
- W3105789788 cites W2096911128 @default.
- W3105789788 cites W2101150949 @default.
- W3105789788 cites W2104085121 @default.
- W3105789788 cites W2116344101 @default.
- W3105789788 cites W2127392678 @default.
- W3105789788 cites W2138049679 @default.
- W3105789788 cites W2146989730 @default.
- W3105789788 cites W2152774008 @default.
- W3105789788 cites W2159504674 @default.
- W3105789788 cites W2163812193 @default.
- W3105789788 cites W2212612681 @default.
- W3105789788 cites W2239370459 @default.
- W3105789788 cites W2240844425 @default.
- W3105789788 cites W2285868373 @default.
- W3105789788 cites W2328436769 @default.
- W3105789788 cites W2467835313 @default.
- W3105789788 cites W2484525193 @default.
- W3105789788 cites W2498126760 @default.
- W3105789788 cites W2525127206 @default.
- W3105789788 cites W2558787751 @default.
- W3105789788 cites W2577179443 @default.
- W3105789788 cites W3037031488 @default.
- W3105789788 cites W3097978841 @default.
- W3105789788 cites W3098567878 @default.
- W3105789788 cites W3098653497 @default.
- W3105789788 cites W3098962958 @default.
- W3105789788 cites W3099116630 @default.
- W3105789788 cites W3099697100 @default.
- W3105789788 cites W3100288267 @default.
- W3105789788 cites W3102109212 @default.
- W3105789788 cites W3102119950 @default.
- W3105789788 cites W3102315646 @default.
- W3105789788 cites W3102337957 @default.
- W3105789788 cites W3102364836 @default.
- W3105789788 cites W3102708276 @default.
- W3105789788 cites W3102935361 @default.
- W3105789788 cites W3103082627 @default.
- W3105789788 cites W3103360303 @default.
- W3105789788 cites W3103584955 @default.
- W3105789788 cites W3103829404 @default.
- W3105789788 cites W3104084565 @default.
- W3105789788 cites W3104181005 @default.
- W3105789788 cites W3105719593 @default.
- W3105789788 cites W3105754030 @default.
- W3105789788 cites W3106126718 @default.
- W3105789788 cites W95632374 @default.
- W3105789788 doi "https://doi.org/10.3847/1538-4357/aa73d9" @default.
- W3105789788 hasPublicationYear "2017" @default.
- W3105789788 type Work @default.
- W3105789788 sameAs 3105789788 @default.
- W3105789788 citedByCount "39" @default.
- W3105789788 countsByYear W31057897882016 @default.
- W3105789788 countsByYear W31057897882017 @default.
- W3105789788 countsByYear W31057897882018 @default.
- W3105789788 countsByYear W31057897882019 @default.
- W3105789788 countsByYear W31057897882020 @default.
- W3105789788 countsByYear W31057897882021 @default.
- W3105789788 countsByYear W31057897882022 @default.
- W3105789788 countsByYear W31057897882023 @default.
- W3105789788 crossrefType "journal-article" @default.
- W3105789788 hasAuthorship W3105789788A5003038198 @default.